Twin Worlds, Divergent Fates: How Obliquity has Differently Shaped Pluto’s and Triton’s Landscapes and Climates
Triton and Pluto are believed to share a common origin, both forming initially in the Kuiper Belt but Triton being later captured by Neptune. Both objects display similar sizes, densities, and atmospheric and surface ice composition, with the presence of volatile ices N2, CH4 and CO. Yet their appearance, including their surface albedo and ice distribution strongly differ.
What can explain these different appearances? A first disparity is that Triton is experiencing significant tidal heating due to its orbit around Neptune, with subsequent resurfacing and a relatively flat surface, while Pluto is not tidally activated and displays a pronounced topography.
Here we present long-term volatile transport simulations of Pluto and Triton, using the same initial conditions and volatile inventory, but with the known orbit and rotation of each object. The model reproduces, to first order, the observed volatile ice surface distribution on Pluto and Triton.
Our results unambiguously demonstrate that obliquity is the main driver of the differences in surface appearance and in climate properties on Pluto and Triton, and give further support to the hypothesis that both objects had a common origin followed by a different dynamical history.
Tanguy Bertrand, François Forget, Emmanuel Lellouch
Comments: 16 pages, 3 figures
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2409.01122 [astro-ph.EP] (or arXiv:2409.01122v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2409.01122
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Journal reference: PNAS, August 12, 2024, 121 (34) e2408226121
Related DOI:
https://doi.org/10.1073/pnas.2408226121
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Submission history
From: Tanguy Bertrand
[v1] Mon, 2 Sep 2024 09:58:00 UTC (1,093 KB)
https://arxiv.org/abs/2409.01122
Astrobiology
